The height variation of granular and oscillatory velocities
Creators
- 1. Sacramento Peak Observatory, Air Force Geophysics Laboratory, Sunspot, N.M. 88349, USA
Description
Previous observations of spatially-resolved vertical velocity variations in ten lines of Fe I spanning the height range 0 < approximately h < approximately 1000 km are re-analyzed using velocity weighting functions. The amplitudes and scale heights of granular and oscillatory velocities are determined, as well as those of the remaining unresolved velocities. It is found that the optimal representation of the amplitude of the outward-decreasing granular velocities is an exponentially decreasing function of height, with a scale height of 150 km and a velocity at zero height of 1.27 km s-1. The optimal representation of the same quantities for oscillatory velocities is an exponential increase with height, with a scale height of 1100 km and a velocity at zero height of 0.35 km s-1. The remaining unresolved velocities decrease with height, with a scale height of 380 km and a velocity at zero height of 2.3 km s-1. (Auth.)
Additional details
Identifiers
- DOI
- 10.1007/bf00155287;
Publishing Information
- Journal Title
- Solar Physics
- Journal Volume
- 50
- Journal Issue
- 2
- Series
- Sol. Phys.
- Journal Page Range
- 239-254
- ISSN
- 0038-0938
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 8316842
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- AMPLITUDES; CHROMOSPHERE; EMISSION SPECTRA; HEIGHT; IRON; OSCILLATIONS; PHOTOSPHERE; SOLAR GRANULATION; SUN; VARIATIONS; VELOCITY; VISIBLE RADIATION; WEIGHTING FUNCTIONS
- Descriptors DEC
- DIMENSIONS; ELECTROMAGNETIC RADIATION; ELEMENTS; FUNCTIONS; METALS; RADIATIONS; SOLAR ACTIVITY; SPECTRA; STARS; TRANSITION ELEMENTS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent